Broad and Narrow Beam Attenuation of 500- to 1,400-Kv. X-Rays in Lead and Concrete

Radiology ◽  
1948 ◽  
Vol 51 (6) ◽  
pp. 849-859 ◽  
Author(s):  
Harold O. Wyckoff ◽  
R. J. Kennedy ◽  
W. R. Bradford
Keyword(s):  
X Rays ◽  
1948 ◽  
Vol 41 (3) ◽  
pp. 223 ◽  
Author(s):  
Harold O. Wyckoff ◽  
Robert J. Kennedy ◽  
William R. Bradford
Keyword(s):  
X Rays ◽  

2010 ◽  
Vol 9 (4) ◽  
pp. 223-236 ◽  
Author(s):  
Fayez H.H. Al-Ghorabie ◽  
Saud S.H. Al-Lyhiani ◽  
Sameer S.A. Natto

AbstractA computer user-code (TRANSMIT), based on the use of the EGSnrc Monte Carlo system, was developed to simulate the transmission of megavoltage x-rays through three different materials used for shielding purposes in radiotherapy. These materials are Lipowitz’s metal, lead and Rad-block. The simulations were performed for 4, 6 and 10 MV x-rays using narrow beam geometry in air. The linear attenuation coefficients, in cm–1, obtained from the simulated transmission curves for Lipowitz’s metal were 0.494, 0.470 and 0.452 for 4, 6 and 10 MV, respectively. For lead, the linear attenuation coefficients were 0.532, 0.507 and 0.483 for 4, 6 and 10 MV, respectively. For Rad-block, the linear attenuation coefficients were 0.561, 0.537 and 0.518 for 4, 6 and 10 MV, respectively. Comparison of the simulation results with experimental results reported in the literature gave a percent deviation <5% which indicates the validity of the simulation results. In addition, broad beam geometry calculations were performed for a variety of field sizes (10 × 10 cm2, 20 × 20 cm2 and 40 × 40 cm2) using the three different attenuators. The results showed that broad beam attenuation coefficients decreased with increased field size and photon energy. For Lipowitz’s metal, the difference in the linear attenuation coefficient data between the broad beam attenuation coefficient and the narrow beam value lies between 3.6% and 20% depending on x-ray energy and field size. Similarly, the difference between the broad beam attenuation coefficient and the narrow beam value for lead lies between 1.5% and 10.4%. For the Rad-block material, the difference lies between 0.53% and 6.8%.


In a former communication to the Royal Society, an attempt was made to determine for certain crystals the exact nature of the diffracting system which produces the Laue X-ray diffraction photographs. The crystals chosen for particular investigation were the isomorphous alkaline halides NaCl, KCl, KBr, and KI. As in the original experiments of Laue and his collaborators, a thin section of crystal was placed in the path of a narrow beam of X-rays, and the radiation diffracted by the crystal made its impression on a photographic plate. By noticing what differences were caused in the photograph by the substitution of heavier for lighter atoms in the crystal, a definite arrangement was decided on as that of the diffracting points of the crystalline grating. Though it was found possible in the case of these simple salts to determine the position of the atoms of alkaline metal and halogen, which constitute the elements of the dimensional diffraction grating, yet this method, which may be called the photographic method, is very limited in its range of applications. It was only the extremely simple nature of the NaCI structure which made its analysis possible. On the other hand, the X-ray spectrometer, which has been devised by W. H. Bragg for the purpose of studying the reflection of X-rays by crystals, affords a very much more powerful method of research into the structure of the crystal.


Living cells grown in tissue culture have been irradiated with a narrow beam of soft X-rays of effective diameter 2·5 μ. The method has been used in conjunction with quantitative ultra-violet photomicrography to investigate the role of the nucleolus in nucleic acid synthesis. The results show that X-irradiation of the nucleolus reduces the amount of nucleic acid synthesized in the nucleus when measured 3 to 7 h after irradiation, whereas X-irradiation of the nuclear sap with an equal dose does not show this effect. The significance of this is discussed.


1987 ◽  
Vol 14 (1) ◽  
pp. 135-139 ◽  
Author(s):  
Ellen E. El-Khatib ◽  
Ervin B. Podgorsak ◽  
Conrado Pla

The present paper deals with the results obtained in the investigation of the atomic structure of rutile and cassiterite by the X-ray spectrometer. A detailed account of the method has been given by Prof. Bragg and his son, W. L. Bragg, in a series of papers communicated to the Royal Society. It consists essentially in allowing a narrow beam of monochromatic X-rays—in this case the rhodium rays—to fall on the face of the crystals, mounted on a spectrometer table, the axis of rotation of which passes through the face of the crystal. The beam is “reflected” by the atom planes parallel to this face, and thence passes into an ionisation chamber, containing methyl bromide in order to increase the ionisation current. The setting of crystal and chamber with regard to the incident beam corresponds to that for which ordinary light is reflected.


2019 ◽  
Vol 71 (Supplement_1) ◽  
Author(s):  
Shuro Takano ◽  
Taku Nakajima ◽  
Kotaro Kohno

AbstractWe present observational data of a molecular line survey toward the nearby galaxies NGC 1068, NGC 253, and IC 342 at wavelengths of 3 mm (∼85–116 GHz) obtained with the Nobeyama 45 m radio telescope. Regarding IC 342, a line survey with high spectral resolution in the 3 mm region was reported for the first time. NGC 1068 is a nearby gas-rich galaxy with X-rays from an active galactic nucleus (AGN), and NGC 253 and IC 342 are nearby gas-rich galaxies with prototypical starbursts. These galaxies are useful for studying the impacts of X-rays and ultraviolet radiation on molecular abundances. The survey was carried out with a resulting rms noise level of a few mK ($T\rm {_A^*}$). As a result we could obtain almost complete data of these galaxies in the 3 mm region: we detected 19–23 molecular species, depending on the galaxies, including several new detections (e.g., cyclic-C3H2 in IC 342). We found that the intensities of HCN, CN, and HC3N relative to 13CO are significantly strong in NGC 1068 compared with those in NGC 253 and IC 342. On the other hand, CH3CCH was not detected in NGC 1068. We obtained these results with the narrow beam (${15{^{\prime\prime}_{.}}2}$–${19{^{\prime\prime}_{.}}1}$) of the 45 m telescope, among single-dish telescopes, and in particular selectively observed molecular gas close to the circumnuclear disk (CND) in NGC 1068. The present line intensities in NGC 1068 were compared with those obtained with the IRAM 30 m radio telescope already reported. As a result, the intensity ratio of each line was found to have information on the spatial distribution. Our observations revealed the line intensities and stringent constraints on the upper limit for the three galaxies with such a narrow beam; consequently, the present data will be a basis for further observations with high spatial resolution.


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